Avtory i prava: Vakuumirovannyi teleskop,
Nacional'naya Solnechnaya observatoriya,
Nacional'naya opticheskaya astronomicheskaya observatoriya
Nacional'naya opticheskaya astronomicheskaya observatoriya
Perevod: Kozyreva A.V.
Poyasnenie:
Kakim obrazom nebol'shie uchastki Solnca mogut vyglyadet' slegka temnee?
Na kartinke vy vidite solnechnoe pyatno - mesto,
gde Solnce nemnogo holodnee i menee
yarkoe po sravneniyu s ostal'noi poverhnost'yu.
Slozhnoe
magnitnoe
pole
Solnca prepyatstvuet perenosu goryachego veshestva, iz-za chego i
obrazuyutsya holodnye oblasti -
pyatna.
Solnechnye
pyatna mogut byt' bol'she, chem Zemlya,
i vremya ih zhizni ogranichivaetsya lish' neskol'kimi dnyami.
Pri vzglyade na
eto izobrazhenie, sdelannoe
s udivitel'no vysokim razresheniem,
horosho vidno, chto poverhnost' Solnca predstavlyaet soboi burlyashee more yacheek
goryachego gaza.
Eti yacheiki nazyvayutsya
granulami.
Razmer solnechnyh
granul
sostavlyaet okolo tysyachi kilometrov, i zhivut oni okolo 10 minut, po istechenii kotoryh
mnogie
granuly lopayutsya.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Publikacii s klyuchevymi slovami:
sunspot - Sun - magnetic field - magnitnoe pole Solnca - Solnechnye pyatna - Solnce - granulyaciya, solnechnaya
Publikacii so slovami: sunspot - Sun - magnetic field - magnitnoe pole Solnca - Solnechnye pyatna - Solnce - granulyaciya, solnechnaya | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
